“Electron acceleration and hard X-ray emission from SOL2013-11-09,” by Yuri Tsap and Galina Motorina. Testing the thick-target model in an interesting flare!
See
http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets
listing the current series, 2008-present, and
http://sprg.ssl.berkeley.edu/~tohban/nuggets/
for the original series, 2005-2008.
We publish these at roughly two-week intervals and welcome contributions,
which should be related, at least loosely, to RHESSI science.
MAX MILLENNIUM NEWS
04 May 2016
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
=====================================================================
1. E-PRINTS POSTED IN THE PAST WEEK
===================================
> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
Spectroscopic Diagnostics of Solar Magnetic Flux Ropes Using Iron
Forbidden Line
-- X. Cheng and M. D. Ding
Transverse oscillations and stability of prominences in a magnetic
field dip
-- D.Y. Kolotkov, G. Nistico and V.M. Nakariakov
Comparing SSN Index to X-ray Flare and Coronal Mass Ejection
Rates from Solar Cycles 22-24
-- Lisa M. Winter, Rick Pernak, and K.S. Balasubramaniam
Quasi-periodic processes in the flare loop generated by sudden
temperature enhancements at loop footpoints
-- M. Karlicky and P. Jelinek
The apparent critical decay index at the onset of solar prominence
eruptions
-- Zuccarello F.P., Aulanier G., Gilchrist S.A.
2. FROM THE EDITOR
==================
The Max Millennium program exists to enhance all aspects of solar
activity research. If you have news that is of broad interest to that
community, feel free to send your message to the MMScience e-mail
list:
http://solar.physics.montana.edu/max_millennium/mmlists.shtml
Address questions to richard.canfield at montana.edu
First Circular
Solar Physics with Radio Observations
- Continued Operation of Nobeyama Radioheliograph -
http://st4a.stelab.nagoya-u.ac.jp/SPRO2016/
Date: September 9 (Fri.) and 10 (Sat.), 2016
Venue: Nagoya University
Access: http://en.nagoya-u.ac.jp/access/index.html
Campus map: http://en.nagoya-u.ac.jp/map/index.html
SOC: K. S. Cho, N. Gopalswamy, M. Ishii, S. Masuda, K. Shibasaki
(chair), and Y. Yan
LOC: S. Masuda (chair), ISEE staff
Objective of the meeting:
Nobeyama Radioheliograph (NoRH) has been observing the Sun since 1992.
After March 2015, International Consortium for the Continued Operation
of Nobeyama Radioheliograph (ICCON) took over the operation from NAOJ
and operated successfully for more than one year. To enhance science
output from NoRH, we wish to organize a symposium to discuss new science
results from NoRH and future targets of NoRH. Recently, many new radio
telescopes started solar observations. This symposium is also a good
chance to learn about them and to discuss collaboration with NoRH.
Deadlines for abstract submission and registration:
July 31, 2016
http://st4a.stelab.nagoya-u.ac.jp/SPRO2016/
Sponsors:
ICCON, ISEE (Nagoya U.)
--
-----------------------------------
Kiyoto Shibasaki
Solar Physics Research Inc.
shibasaki.kiyoto(a)md.ccnw.ne.jp
http://www.md.ccnw.ne.jp/sprinc/
-----------------------------------
No. 271, “Radio polarization signatures in twisted flare loops” by Ivan Sharykin and Alexei Kuznetsov: Flux-rope geometry via radio polarization signs
No. 272, “Extreme events, stellar evolution, and magnetic reconnection” by Hugh Hudson: Stellar activity measured by flare rates over the eons.
See
http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets
listing the current series, 2008-present, and
http://sprg.ssl.berkeley.edu/~tohban/nuggets/
for the original series, 2005-2008.
We publish these at roughly two-week intervals and welcome contributions,
which should be related, at least loosely, to RHESSI science.
MAX MILLENNIUM NEWS
27 April 2016
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
=====================================================================
1. E-PRINTS POSTED IN THE PAST WEEK
===================================
> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
Temporal Offsets between Maximum CME Speed Index and Solar, Geomagnetic,
and Interplanetary Indicators during Solar Cycle 23 and the Ascending
Phase of Cycle 24
-- A. Ozguc, A. Kilcik, K. Georgieva, B. Kirov
2. FROM THE EDITOR
==================
The Max Millennium program exists to enhance all aspects of solar
activity research. If you have news that is of broad interest to that
community, feel free to send your message to the MMScience e-mail
list:
http://solar.physics.montana.edu/max_millennium/mmlists.shtml
Address questions to richard.canfield at montana.edu
MAX MILLENNIUM NEWS
20 April 2016
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
=====================================================================
1. E-PRINTS POSTED IN THE PAST WEEK
===================================
> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
Constraints on energy release in solar flares from RHESSI and GOES
X-ray observations. II. Energetics and energy partition
-- Warmuth, A., Mann, G.
Constraints on energy release in solar flares from RHESSI and GOES
X-ray observations I. Physical parameters and scalings
-- Warmuth, A., Mann, G.
Modelling of Nonthermal Microwave Emission From Twisted Magnetic
Loops
-- I. N. Sharykin, A. A. Kuznetsov
Unprecedented Fine Structure of a Solar Flare Revealed by the 1.6m
New Solar Telescope
-- Ju Jing, Yan Xu, Wenda Cao, Chang Liu, Dale Gary & Haimin Wang
The Nature of CME-Flare Associated Coronal Dimming
-- J. X. Cheng, J. Qiu
Long Duration Flare Emission: Impulsive Heating or Gradual Heating?
-- Qiu, Jiong, Longcope, Dana, W.
Lifecycle of a large-scale polar coronal pseudostreamer/cavity
system
-- Chloe Guennou , Laurel A. Rachmeler, Daniel B. Seaton and
Frederic Auchere
Amended results for hard X-ray emission by non-thermal thick target
recombination in solar flares
-- Reep, J.W. & Brown, J.C.
The instability and non-existence of multi-stranded loops, when
driven by transverse waves
-- N. Magyar, T. Van Doorsselaere
2. FROM THE EDITOR
==================
The Max Millennium program exists to enhance all aspects of solar
activity research. If you have news that is of broad interest to that
community, feel free to send your message to the MMScience e-mail
list:
http://solar.physics.montana.edu/max_millennium/mmlists.shtml
Address questions to richard.canfield at montana.edu
MAX MILLENNIUM NEWS
13 April 2016
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
=====================================================================
1. E-PRINTS POSTED IN THE PAST WEEK
-----------------------------------
> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
On the origin of 140 GHz emission from the 4 July 2012 solar flare
-- Yuriy T. Tsap, Victoria V. Smirnova, Alexander S. Morgachev,
Galina G. Motorina, Eduard P. Kontar, Valery G. Nagnibeda,
Polina V. Strekalova
Light walls around sunspots observed by the Interface Region
Imaging Spectrograph
-- Y. J. Hou, T. Li, S. H. Yang and J. Zhang
2. FROM THE EDITOR
------------------
The Max Millennium program exists to enhance all aspects of solar
flare research. If you have news that is of broad interest to that
community, feel free to send your message to the MMScience e-mail list:
http://solar.physics.montana.edu/max_millennium/mmlists.shtml
Address questions to canfield at physics.montana.edu
MAX MILLENNIUM NEWS
06 April 2016
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
=====================================================================
1. E-PRINTS POSTED IN THE PAST WEEK
===================================
> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
Stereoscopic Observation of Slipping Reconnection in A Double
Candle-Flame-Shaped Solar Flare
-- Tingyu Gou, Rui Liu, Yuming Wang, Kai Liu, Bin Zhuang, Jun
Chen,Quanhao Zhang, and Jiajia Liu
A Tiny Eruptive Filament as a Flux-Rope Progenitor and Driver
of a Large-Scale CME and Wave
-- V.V. Grechnev, A.M. Uralov, A.A. Kochanov, I.V. Kuzmenko,
D.V. Prosovetsky, Ya.I. Egorov, V.G. Fainshtein, L.K. Kashapova
Active Latitude Oscillations Observed on the Sun
-- A. Kilcik, V. Yurchyshyn, F. Clette, A. Ozguc, J.-P. Rozelot
Stochastic transients as a source of quasi-periodic processes
in the solar atmosphere
-- Ding Yuan, Jiangtao Su, Fangran Jiao, Robert W. Walsh
2. FROM THE EDITOR
==================
The Max Millennium program exists to enhance all aspects of solar
activity research. If you have news that is of broad interest to that
community, feel free to send your message to the MMScience e-mail
list:
http://solar.physics.montana.edu/max_millennium/mmlists.shtml
Address questions to richard.canfield at montana.edu
MAX MILLENNIUM NEWS
30 March 2016
CONTENTS
1. E-PRINTS POSTED IN THE PAST WEEK
2. FROM THE EDITOR
=====================================================================
1. E-PRINTS POSTED IN THE PAST WEEK
===================================
> http://solar.physics.montana.edu/cgi-bin/eprint/default_page.pl
Suppression of parallel transport in turbulent magnetized plasmas
and its impact on non-thermal and thermal aspects of solar flares
-- Bian, Nicolas H., Kontar, Eduard P., and Emslie, A. Gordon
The First X-ray Imaging Spectroscopy of Quiescent Solar Active
Regions with NuSTAR
-- Iain G. Hannah, Brian W. Grefenstette, David M. Smith, Lindsay
Glesener, Sam Krucker, Hugh S. Hudson, Kristin K. Madsen,
Andrew Marsh, Stephen M. White, Amir Caspi, Albert Y. Shih, Fiona
A. Harrison, Daniel Stern, Steven E. Boggs, Finn E. Christensen,
William W. Craig, Charles J. Hailey, William W. Zhang
Hooked flare ribbons and flux-rope related QSL footprints
-- Jie Zhao, Stuart A. Gilchrist, Guillaume Aulanier, Brigitte
Schmieder, Etienne Pariat, Hui Li
Hi-C Observations of Sunspot Penumbral Bright Dots
-- Shane E. Alpert, Sanjiv K. Tiwari, Ronald L. Moore, Amy
R. Winebarger, Sabrina L. Savage
Predicting Coronal Mass Ejections Using Machine Learning Methods
-- Monica G. Bobra and Stathis Ilondis
2. FROM THE EDITOR
==================
The Max Millennium program exists to enhance all aspects of solar
activity research. If you have news that is of broad interest to that
community, feel free to send your message to the MMScience e-mail
list:
http://solar.physics.montana.edu/max_millennium/mmlists.shtml
Address questions to richard.canfield at montana.edu